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The primary goal of EXIST is to find black holes in the local and distant universe.
It is thus clear that GOODS will generate the deepest, largest and most uniform panchromatic data-set to study the distant universe.
They also will be scouring the distant universe to discern the properties of the hypothesized substance known as dark energy.
This star's motion with respect to "fixed points" in the distant universe thus needed to be measured independently.
Looking back in time at the distant universe, these supermassive black holes appear as very bright quasars.
The most powerful way of doing this is to measure the masses of galaxy clusters, particularly those in the distant Universe.
For the past several years, we have been observing a new spectroscopic survey of the distant Universe, the DEIMOS/DEEP redshift survey.
Light from our own galaxy billions of years ago has long since left the galaxy and is traveling throughout the distant Universe.
We successfully tracked the black hole and galaxy growth in the distant universe with NASA's Chandra, Hubble, Spitzer, and other observatories.
The latest result involves the development of a new method to determine distances to quasars, rapidly growing black holes in the distant Universe that shine extremely brightly.
"We will be able to probe questions about dark matter and dark energy and make a 3-D map of the distant Universe," Strauss said.
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